| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 94.64 | 480.90 | 79.88 | 407.60 | -13.66 | 120.54 | -51.49 | 110.29 | 0.8122 | 369.4 | 161.4 | |
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back to the solar disc SDO HMI 2011-11-03 05:58:59 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.83 | 258.05 | 5.42 | 206.95 | -14.90 | 123.93 | -48.10 | 112.88 | 0.7830 | 1011.1 | 287.5 | |
| 2.25 | -1.00 | 1.78 | -1.00 | -14.58 | 123.97 | -48.05 | 112.51 | 0.7815 | 1048.0 | 999999 | |
| 10.12 | -1.00 | 8.14 | -1.00 | -15.49 | 123.42 | -48.61 | 113.41 | 0.7901 | 711.8 | 999999 | |
| 21.54 | -1.00 | 17.28 | -1.00 | -14.90 | 123.37 | -48.66 | 112.67 | 0.7886 | 768.7 | 999999 | |
| 1.56 | -1.00 | 1.26 | -1.00 | -15.38 | 123.12 | -48.91 | 113.16 | 0.7926 | 448.9 | 999999 | |
| 6.75 | -1.00 | 5.42 | -1.00 | -14.44 | 123.13 | -48.90 | 112.03 | 0.7895 | 725.7 | 999999 | |
| 1.82 | -1.00 | 1.47 | -1.00 | -14.56 | 122.77 | -49.26 | 112.04 | 0.7935 | 516.0 | 999999 | |
| 0.87 | -1.00 | 0.70 | -1.00 | -14.72 | 122.72 | -49.31 | 112.21 | 0.7944 | 175.7 | 999999 | |
| 0.00 | 0.87 | 0.00 | 0.71 | -13.89 | 121.97 | -50.06 | 110.94 | 0.7993 | 473.0 | 390.9 | |
| 0.00 | 3.81 | 0.00 | 3.15 | -14.31 | 121.65 | -50.38 | 111.34 | 0.8036 | 337.0 | 313.9 | |
| 1.30 | 2.42 | 1.08 | 2.02 | -14.11 | 121.37 | -50.66 | 111.01 | 0.8057 | 348.8 | 242.3 | |
| 0.00 | 0.87 | 0.00 | 0.72 | -13.91 | 121.09 | -50.94 | 110.67 | 0.8078 | -332.0 | -261.7 | |
| 3.37 | 4.41 | 2.82 | 3.68 | -13.69 | 121.06 | -50.97 | 110.40 | 0.8075 | 429.8 | 287.8 | |
| 1.21 | 7.35 | 1.06 | 6.38 | -13.31 | 119.13 | -52.90 | 109.34 | 0.8248 | -554.4 | -620.9 | |
| 5.02 | 8.65 | 4.47 | 7.69 | -14.56 | 118.56 | -53.47 | 110.63 | 0.8332 | -716.1 | -554.5 | |
| 0.00 | 0.95 | 0.00 | 0.85 | -13.49 | 118.19 | -53.84 | 109.28 | 0.8339 | -517.0 | -423.9 | |
| 0.00 | 2.25 | 0.00 | 2.06 | -14.75 | 117.43 | -54.60 | 110.51 | 0.8437 | -708.0 | -631.3 | |
| 2.08 | 14.79 | 1.92 | 13.71 | -15.11 | 117.24 | -54.79 | 110.86 | 0.8462 | -757.7 | -579.6 | |
| 0.00 | 1.99 | 0.00 | 1.83 | -14.54 | 117.24 | -54.79 | 110.22 | 0.8449 | -724.0 | -660.5 | |
| 0.00 | 1.21 | 0.00 | 1.12 | -14.87 | 117.07 | -54.96 | 110.53 | 0.8472 | -540.0 | -430.1 | |
| 4.15 | -18.00 | 3.87 | -18.00 | -15.19 | 116.89 | -55.14 | 110.85 | 0.8495 | -433.0 | 999999 | |
| 0.00 | 1.04 | 0.00 | 0.95 | -14.10 | 117.30 | -54.73 | 109.73 | 0.8434 | -428.0 | -401.0 | |
| 8.22 | 129.68 | 7.24 | 115.32 | -10.99 | 118.11 | -53.92 | 106.33 | 0.8289 | 960.3 | 220.3 | |
| 2.85 | 5.10 | 2.63 | 4.70 | -13.84 | 117.07 | -54.96 | 109.35 | 0.8448 | -581.8 | -577.2 | |
| 0.00 | 1.30 | 0.00 | 1.20 | -14.22 | 116.93 | -55.10 | 109.75 | 0.8468 | -450.0 | -414.1 | |
| 0.00 | 17.04 | 0.00 | 16.15 | -15.35 | 116.33 | -55.70 | 110.87 | 0.8546 | -231.0 | -219.0 | |
| 0.00 | 0.95 | 0.00 | 0.96 | -18.02 | 115.00 | -57.03 | 113.47 | 0.8717 | -444.0 | -476.5 | |
| 11.42 | -23.00 | 10.21 | -23.00 | -10.97 | 117.49 | -54.54 | 106.14 | 0.8346 | 557.3 | 999999 | |
| 1.38 | 6.49 | 1.30 | 6.13 | -14.38 | 116.33 | -55.70 | 109.77 | 0.8525 | -270.0 | -113.5 | |
| 0.00 | 1.64 | 0.00 | 1.63 | -14.86 | 114.62 | -57.41 | 109.84 | 0.8678 | -355.0 | -357.1 | |
| 0.00 | 1.12 | 0.00 | 1.13 | -15.51 | 114.34 | -57.69 | 110.49 | 0.8714 | -214.0 | -285.7 | |
| 0.00 | 1.04 | 0.00 | 0.96 | -10.20 | 116.10 | -55.93 | 104.90 | 0.8458 | 502.0 | 440.2 | |
| 1.90 | 5.02 | 1.81 | 4.78 | -10.30 | 114.97 | -57.06 | 104.75 | 0.8560 | 518.7 | 460.0 | |
| 0.00 | 1.82 | 0.00 | 1.80 | -9.81 | 113.45 | -58.58 | 103.86 | 0.8682 | 417.0 | 339.1 | |
| 0.00 | 1.04 | 0.00 | 1.02 | -8.83 | 113.54 | -58.49 | 102.77 | 0.8659 | 458.0 | 366.8 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |